Depth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above 10(17.8) eV

By A. Aab, A. Aminaei, S. Buitink, S. Jong, Heino Falcke, S. Grebe, J. Hörandel, S. Jansen, A. Nelles, H. Schoorlemmer and 6 more. 2014

338 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/b092fe54ad3cb6a17d66242f6c06ed2f3f2100f3

How researchers see this paper

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In Astronomy and Astrophysics

1. Tim Huege
2. G. Farrar
3. J. Biteau
4. Ralph Engel
5. M. Unger
6. Angela V. Olinto
7. R. Ulrich
8. A. V. Vliet

In Nuclear and High Energy Physics

1. Tim Huege
2. Angela V. Olinto
3. K. Kampert
4. M. Unger
5. Ralph Engel
6. G. Farrar
7. J. Biteau
8. R. Ulrich

Citations in the corpus

• Depth of Ultra High Energy Cosmic Ray Induced Air Shower Maxima Measured by the Telescope Array Black Rock and Long Ridge FADC Fluorescence Detectors and Surface Array in Hybrid Mode (2018, methodology): “Auger has shown an energy evolution in 〈Xmax〉 and σ(Xmax) to heavier primaries above 1018.3 eV (Aab et al. 2014).”
• Combined fit of spectrum and composition data as measured by the Pierre Auger Observatory (2016, methodology): “2) and Xmax distributions [5] (in bins of 20 g/cm(2)) in the same bins of energy up to log10(E/eV) = 19.”